Abstract
We propose a simple but effective mechanism to realize an inflationary early universe consistent with the observed WMAP, Planck and/or BICEP2 data, which would be incorporated in various supersymmetric models of elementary particles constructed in the (effective) five-dimensional spacetime. In our scenario, the inflaton field is identified with one of the moduli appearing when the fifth direction is compactified, and a successful cosmological inflation without the so-called η problem can be achieved by a very simple moduli stabilization potential. We also discuss the related particle cosmology during and (just) after the inflation, such as the (no) cosmological moduli problem.
| Original language | English |
|---|---|
| Article number | 027 |
| Journal | Journal of Cosmology and Astroparticle Physics |
| Volume | 2014 |
| Issue number | 11 |
| DOIs | |
| Publication status | Published - 2014 Nov 1 |
Fingerprint
Keywords
- cosmological applications of theories with extra dimensions
- inflation
- string theory and cosmology
- supersymmetry and cosmology
ASJC Scopus subject areas
- Astronomy and Astrophysics
Cite this
Moduli inflation in five-dimensional supergravity models. / Abe, Hiroyuki; Otsuka, Hajime.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2014, No. 11, 027, 01.11.2014.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Moduli inflation in five-dimensional supergravity models
AU - Abe, Hiroyuki
AU - Otsuka, Hajime
PY - 2014/11/1
Y1 - 2014/11/1
N2 - We propose a simple but effective mechanism to realize an inflationary early universe consistent with the observed WMAP, Planck and/or BICEP2 data, which would be incorporated in various supersymmetric models of elementary particles constructed in the (effective) five-dimensional spacetime. In our scenario, the inflaton field is identified with one of the moduli appearing when the fifth direction is compactified, and a successful cosmological inflation without the so-called η problem can be achieved by a very simple moduli stabilization potential. We also discuss the related particle cosmology during and (just) after the inflation, such as the (no) cosmological moduli problem.
AB - We propose a simple but effective mechanism to realize an inflationary early universe consistent with the observed WMAP, Planck and/or BICEP2 data, which would be incorporated in various supersymmetric models of elementary particles constructed in the (effective) five-dimensional spacetime. In our scenario, the inflaton field is identified with one of the moduli appearing when the fifth direction is compactified, and a successful cosmological inflation without the so-called η problem can be achieved by a very simple moduli stabilization potential. We also discuss the related particle cosmology during and (just) after the inflation, such as the (no) cosmological moduli problem.
KW - cosmological applications of theories with extra dimensions
KW - inflation
KW - string theory and cosmology
KW - supersymmetry and cosmology
UR - http://www.scopus.com/inward/record.url?scp=84914180316&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84914180316&partnerID=8YFLogxK
U2 - 10.1088/1475-7516/2014/11/027
DO - 10.1088/1475-7516/2014/11/027
M3 - Article
AN - SCOPUS:84914180316
VL - 2014
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
SN - 1475-7516
IS - 11
M1 - 027
ER -